Submillimeter H 2 O and H 2 O + emission in lensed ultra- and hyper-luminous infrared galaxies at z ~ 2-4
Journal article, 2016
Radio lines: ISM
ISM: molecules
Galaxies: ISM
Submillimeter: galaxies
Infrared: galaxies
Galaxies: high-redshift
Author
C. Yang
University of Paris-Sud
Pierre and Marie Curie University (UPMC)
Chinese Academy of Sciences
Centre national de la recherche scientifique (CNRS)
A.A. Omont
Centre national de la recherche scientifique (CNRS)
Pierre and Marie Curie University (UPMC)
A. Beelen
University of Paris-Sud
E. Gonzalez-Alfonso
University of Alcalá
R. Neri
Institut de Radioastronomie Millimétrique (IRAM)
Y. Gao
Chinese Academy of Sciences
P. van der Werf
Leiden University
A. Weiß
Max Planck Society
R. Gavazzi
Pierre and Marie Curie University (UPMC)
Centre national de la recherche scientifique (CNRS)
Niklas Falstad
Chalmers, Earth and Space Sciences, Radio Astronomy and Astrophysics
A. J. Baker
Rutgers University
R. S. Bussmann
Cornell University
A. Cooray
University of California at Irvine (UCI)
P. Cox
Atacama Large Millimeter-submillimeter Array (ALMA)
H. Dannerbauer
University of Vienna
S. Dye
University of Nottingham
M. Guélin
Institut de Radioastronomie Millimétrique (IRAM)
R. J. Ivison
European Southern Observatory (ESO)
University of Edinburgh
M. Krips
Institut de Radioastronomie Millimétrique (IRAM)
M. Lehnert
Pierre and Marie Curie University (UPMC)
Centre national de la recherche scientifique (CNRS)
M. J. Michalowski
University of Edinburgh
D. A. Riechers
Cornell University
M. Spaans
University of Groningen
E. Valiante
Cardiff University
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 595 Art no A80- A80Subject Categories
Astronomy, Astrophysics and Cosmology
Roots
Basic sciences
Infrastructure
Onsala Space Observatory
DOI
10.1051/0004-6361/201628160